Solar wind origin in coronal funnels

Science

Volumn 308, Issue 5721, 2005, Pages 519-523

  Tu, Chuan Yi ^a,b   Zhou, Cheng ^a   Marsch, Eckart ^b   Xia, Li Dong ^c   Zhao, Liang ^a   Wang, Jing Xiu ^d   Wilhelm, Klaus ^b  

^a PEKING UNIVERSITY   (China)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^c UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^d CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

[No Author keywords available]

Indexed keywords

CORRELATION METHODS; DOPPLER EFFECT; IONS; MAGNETIC FIELDS; SOLAR SYSTEM; VELOCITY MEASUREMENT; WIND;

CORONAL FUNNELS; MAGNETIC FUNNELS; PHOTOSPHERE; SOLAR WIND;

SOLAR ENERGY;

NEON;

SOLAR WIND;

ALTITUDE; ARTICLE; ASTRONOMY; ATMOSPHERE; CORRELATION ANALYSIS; FORCE; MAGNETIC FIELD; PRIORITY JOURNAL; RADIATION; VELOCITY; WIND;

EID: 17644421463     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1109447     Document Type: Article

References (40)

1. L. Biermann, Zeitschrift für Astrophysik 29, 274 (1951).
2. E. N. Parker, Astrophys. J. 128, 664 (1958).
3. M. Neugebauer, C. W. Snyder, Science 138, 1095 (1962).
4. M. Neugebauer, C. W. Snyder, J. Geophys. Res. 71, 4469 (1966).
5. Y. C. Whang, C. C. Chang, J. Geophys. Res. 70, 4175 (1965).
6. R. E. Hartle, P. A. Sturrock, Astrophys. J. 151, 1155 (1968).
7. A. J. Hundhausen, Coronal Expansion and Solar Wind (Springer-Verlag, Heidelberg, 1972).
8. E. Leer, T. E. Holzer, Solar Phys. 63, 143 (1979).
9. E. Leer, T. E. Holzer, J. Geophys. Res. 85, 4681 (1980).
10. C.-Y. Tu, Solar Phys. 109, 149 (1987).
11. J. V. Hollweg, J. Geophys. Res. 91, 4111 (1986).
12. V. H. Hansteen, E. Leer, J. Geophys. Res. 100, 21577 (1995).
13. C.-Y. Tu, E. Marsch, Solar Phys. 171, 363 (1997).
14. J. F. McKenzie, G. V. Sukhorukova, W. I. Axford, Astron. Astrophys. 330, 1145 (1998).
15. W. I. Axford, J. F. McKenzie, in Solar Wind Seven, E. Marsch and R. Schwenn, Eds., (Pergamon Press, Oxford, 1992), pp. 1-5.
16. W. I. Axford, J. F. McKenzie, in Cosmic Winds and the Heliosphere, J. R. Jokipii, C. P. Sonett, M. S. Giampapa, Eds. (Arizona University Press, Tucson, 1997), pp. 31-66.
17. E. Marsch, C.-Y. Tu, Solar Phys. 176, 87 (1997).
18. P. Hackenberg, E. Marsch, G. Mann, Astron. Astrophys. 360, 1139 (2000).
19. A. H. Gabriel, Philos. Trans. R. Soc. A281, 339 (1976).
20. J. F. Dowdy Jr., A. G. Emslie, R. L. Moore, Solar Phys. 112, 255 (1987).
21. K. Wilhelm et al., Solar Phys. 170, 75 (1997).
22. P. Lemaire et al., Solar Phys. 170, 105 (1997).
23. D. M. Hassler et al., Science 283, 810 (1999).
24. K. Wilhelm, I. E. Dammasch, E. Marsch, D. M. Hassler, Astron. Astrophys. 353, 749 (2000).
25. L. D. Xia, E. Marsch, W. Curdt, Astron. Astrophys. 399, L5 (2003).
26. L. D. Xia, E. Marsch, K. Wilhelm, Astron. Astrophys. 424, 1025 (2004).
27. T. Wiegelmann, T. Neukirch, Solar Phys. 208, 233 (2002).
28. P. H. Scherrer et al., Solar Phys. 162, 129 (1995).
29. E. Marsch, T. Wiegelmann, L. D. Xia, Astron. Astrophys. 428, 629 (2004).
30. Ø. Lie-Svendsen, V. H. Hansteen, E. Leer, Astrophys. J. 596, 621 (2003).
31. J. P. Delaboudinière et al., Solar Phys. 162, 291 (1995).
32. Materials and methods are available as supporting material on Science Online.
33. N. Seehafer, Solar Phys. 58, 215 (1978).
34. H. Peter, Astron. Astrophys. 374, 1108 (2001).
35. H. Peter, B. V. Gudiksen, Å. Nordlund, Astrophys. J. 617, L85 (2004).
36. I. E. Dammasch, K. Wilhelm, W. Curdt, D. M. Hassler, Astron. Astrophys. 346, 285 (1999).
37. T. J. M. Boyd and J. J. Sanderson, Plasma Dynamics (Thomas Nelson and Sons, London, 1969).
38. W. C. Feldman, B. L. Barraclough, J. L. Phillips, Y.-M. Wang, Astron. Astrophys. 316, 355 (1996).
39. L. A. Fisk, J. Geophys. Res. 108, 1157 (2003).
40. The National Natural Science Foundation of China supported C.-Y.T., C.Z., and L. Z. under projects with the contract nos. 40336053, 4017404S and 40436015; J.-X. Wang, contract no. 10233050; and L.-D.X., contract no. 40436015. The foundation Major Project of National Basic Research supported C.-Y.T., C.Z., L-D.X., L. Z., and J.-X.W. under contract no. G-200078405. C.-Y.T. is supported by the Beijing Education Project XK100010404. The SUMER project is financially supported by DLR, CNES, NASA, and the ESA PRODEX program (Swiss contribution). SUMER, EIT, and MDI are instruments on SOHO, an ESA and NASA mission. We thank the teams of MDI and EIT for providing the magnetic field data and the context image.